Migration-driven Planet Growth

Migration-Driven Planet Growth is a theoretical framework in planetary formation that explains the enhancement of planetary core accretion and final mass distribution through the inward or outward orbital migration of protoplanetary embryos, distinguishing it from static in-situ growth models by incorporating dynamical migration effects as a central mechanism for planet assembly.

52

Publications

5.1K

Citations

74

Authors

71

Institutions

Publications per year

2017–2026

24

Authors

74

  1. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    7 publications · 334 citations

    7

    h-index

  2. SN
    Sean N. Raymond

    Laboratoire d'Astrophysique de Bordeaux, France

    6 publications · 1.7K citations

    6

    h-index

  3. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    4 publications · 1.4K citations

    4

    h-index

  4. AI
    André Izidoro

    Centre National de la Recherche Scientifique, France

    4 publications · 265 citations

    4

    h-index

  5. WB
    W. Benz

    University of Bern, Switzerland

    3 publications · 818 citations

    3

    h-index

1–5 of 74

Venues

  1. Astronomy and Astrophysics

    12 publications · 1.4K citations

    12

    h-index

  2. 10

    h-index

  3. Icarus

    6 publications · 338 citations

    6

    h-index

  4. The Astrophysical Journal

    ApJ · 5 publications · 307 citations

    5

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 234 citations

    5

    h-index

1–5